The course describes the theory of planetary orbital dynamics in the context of exoplanet detection and also the characterization of multi-planet systems.

You will learn about celestial mechanics to have a broad knowledge of the important quantities that govern the evolution of a planetary system.
You will also learn how researchers put these principles into play to derive the properties of observed extra-solar planetary systems, to simulate their dynamical evolution of systems and test their stability.
Finally, you will learn about the ways to go beyond the point-mass approximation and the classical Newtonian approach.

The key content and notions addressed include:

  • Celestial Mechanics
  • Numerical integrations
  • Dynamical parameter determination
  • Stability and chaos
  • Tidal interactions 


Where: Room 263

When: Thursday from 08h45 to 10h30 (exercises sessions on Friday from 08h45 to 10h30)
 
Who: Prof. S. Udry, Prof. E. Bolmont


Exams:
Oral exam
Sessions: Jun/Aug-Sep 
ECTS : 4.5